ABSTRACT The Laser Interferometer Space Antenna (LISA) will open the mHz frequency
window of the gravitational-wave (GW) landscape. Among all the new GW sources expected …

Abstract We describe the Dark Energy Survey (DES) photometric data set assembled from
the first three years of science operations to support DES Year 3 cosmologic analyses, and …

We present the final sample of the Exploration of Local VolumE Satellites (ELVES) survey, a
survey of the dwarf satellites of a nearly volume-limited sample of Milky Way (MW)− like …

We report on the host association of FRB 20181030A, a repeating fast radio burst (FRB) with
a low dispersion measure (103.5 pc cm− 3) discovered by the CHIME/FRB Collaboration et …

We present new spectroscopic observations of the diffuse Milky Way satellite galaxies Antlia
2 and Crater 2, taken as part of the Southern Stellar Stream Spectroscopic Survey (S 5). The …

The structure of a dwarf galaxy is an important probe of the effects of stellar feedback and
environment. Using an unprecedented sample of 223 low-mass satellites from the ongoing …

Ultra-diffuse galaxies (UDGs) are the lowest-surface-brightness galaxies known, with typical
stellar masses of dwarf galaxies but sizes similar to those of larger galaxies such as the …

We present a catalog of 5598 ultra-diffuse galaxy (UDG) candidates with effective radius re>
5 farcs 3 distributed throughout the southern portion of the DESI Legacy Imaging Survey …

We present a preview of the faint dwarf galaxy discoveries that will be possible with the Vera
C. Rubin Observatory and Subaru Hyper Suprime-Cam in the next decade. In this work, we …

We use spectral energy distribution (SED) fitting to place constraints on the stellar
population properties of 29 quiescent ultra-diffuse galaxies (UDGs) across different …